Stacked radial profiles of log Age_L, [Fe/H]_L, and A_v. The left panels present the case of the E-MILES SSP models, and the right panels show the case of BC03. Gray open symbols correspond to the stellar population values of each individual bin in each spatially resolved object. Stars have been obtained by averaging the stellar population values of the sample in constant bins of 0.2 R_eff between 0 ≤ R ≤ 3.6 R_eff. The error bars are the standard deviation of the mean. When available, the profiles obtained by CALIFA (González Delgado et al. 2015) have been overplotted. MaNGA (Goddard et al. 2017) for early-type galaxies with log M_⋆> 11.0 was also considered. The dashed black line corresponds to the best linear fit of the average stellar population values (stars).